From the past of meteorites

Details From the past of meteorites From the past of meteorites

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975prir....7...38l&link_type=abstract

From the past of meteorites NASA Transl. into ENGLISH from Priroda (Moscow), no. 7, Jul. 1975 p 38-45

Computer Science

Meteorites, Meteoritic Composition, Origins, Asteroids, Breccia, Cosmology, Meteor Trails

Scientific paper

Studies of the structure and composition of meteorites which have revealed important knowledge of the origin and formation of meteorites are discussed. Such research suggests that meteorites originated initially from asteroids that underwent collisions and disintegrated into smaller fragments. Tracks formed by penetrating solar cosmic rays suggest that meteorites represent consolidated regoliths formed on the surface of the formative bodies. The imputance of the intermixing of meteoritic matter within its body is discussed. The results of studies of recently discovered carbonaceous chondrites also support the theory that meteorites were formed under conditions of balanced condensation of refractory matter in a cooling protoplanetary disc.

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